2017
DOI: 10.1007/jhep07(2017)009
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“1k F ” singularities and finite density ABJM theory at strong coupling

Abstract: We study non-analytic behavior in the static charge susceptibility in finite density states of the ABJM theory using its holographic dual. Emphasis is placed on a particular state characterized by vanishing entropy density at zero temperature, and Fermi surface-like singularities in various fermionic correlation functions. The susceptibility exhibits branch points in the complex momentum plane, with a real part quantitatively very similar to the location of the Fermi surface singularities. arXiv:1612.06823v2 [… Show more

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Cited by 4 publications
(8 citation statements)
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“…The damping rates of the holographic models are of the order of the Fermi momentum, l −1 d = Im(k * ) ∼ k F , whereas in our model we have l −1 d ∼ λ 2 . We consider a dimensionful coupling λ 2 k F whereas the coupling in [33,34] is dimensionless and is taken to infinity, likely more similar to the k F λ 2 case. If we are indeed seeing the same phenomenon then we would expect the damping rate of our model, l −1 d (λ 2 ), to go as λ 2 for λ 2 k F but then saturate to ∼ k F once λ 2 ∼ k F where our theory breaks down.…”
Section: Resultsmentioning
confidence: 99%
“…The damping rates of the holographic models are of the order of the Fermi momentum, l −1 d = Im(k * ) ∼ k F , whereas in our model we have l −1 d ∼ λ 2 . We consider a dimensionful coupling λ 2 k F whereas the coupling in [33,34] is dimensionless and is taken to infinity, likely more similar to the k F λ 2 case. If we are indeed seeing the same phenomenon then we would expect the damping rate of our model, l −1 d (λ 2 ), to go as λ 2 for λ 2 k F but then saturate to ∼ k F once λ 2 ∼ k F where our theory breaks down.…”
Section: Resultsmentioning
confidence: 99%
“…In the former case, exponentially damped Friedel oscillations were uncovered at long distances, apparently at the wavevector where Re[ν − (k)] = 0 (with the expressions appropriate for an AdS×R 2 IR geometry). [45] found that, on the contrary, these oscillations do not survive at long distances in the U (1) 4 black hole, which happens to have an η = 1 IR. This is consistent with the results in [8] that there is no low energy longitudinal spectral weight.…”
Section: Discussionmentioning
confidence: 98%
“…We would like to thank Chris Rosen for very interesting discussions and for sharing with us the results of [45] prior to their publication. We are also grateful to Sean Hartnoll for discussions and comments on a draft.…”
Section: Acknowledgmentsmentioning
confidence: 99%
“…1(b) and φ is a phase constant. The details behind (84) and (86) can be found in Appendix D. The exponential factor on the right hand side of (86) is explicitly in contrast to the case in a weakly-coupled field theory, such type of Friedel-like oscillation with faster than power-law decay behavior is observed in the densitydensity correlation in other holographic strongly-coupled systems [27,33,34] and in the zero fermionic flavor limit: N f → 0 [35].…”
Section: Discussionmentioning
confidence: 99%